Smail, I. and Dudzevičiūtė , U. and Stach, S.M. and Almaini, O. and Birkin, J.E. and Chapman, S.C. and Chen, C.-C. and Geach, J.E. and Gullberg, B. and Hodge, J.A. and Ikarashi, S. and Ivison, R.J. and Scott, D. and Simpson, C. and Swinbank, A.M. and Thomson, A.P. and Walter, F. and Wardlow, J.L. and van der Werf, P. (2021) 'An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies.', Monthly Notices of the Royal Astronomical Society, 502 (3). pp. 3426-3435.
We analyse a robust sample of 30 near-infrared-faint (KAB > 25.3, 5σ) submillimetre galaxies (SMGs) selected from a 0.96 deg2 field to investigate their properties and the cause of their faintness in optical/near-infrared wavebands. Our analysis exploits precise identifications based on Atacama Large Millimeter Array (ALMA) 870-μm continuum imaging, combined with very deep near-infrared imaging from the UKIDSS Ultra Deep Survey. We estimate that SMGs with KAB > 25.3 mag represent 15 ± 2 per cent of the total population brighter than S870 = 3.6 mJy, with a potential surface density of ∼450 deg−2 above S870 ≥ 1 mJy. As such, they pose a source of contamination in surveys for both high-redshift ‘quiescent’ galaxies and very high redshift Lyman-break galaxies. We show that these K-faint SMGs represent the tail of the broader submillimetre population, with comparable dust and stellar masses to KAB ≤ 25.3 mag SMGs, but lying at significantly higher redshifts (z = 3.44 ± 0.06 versus z = 2.36 ± 0.11) and having higher dust attenuation (AV = 5.2 ± 0.3 versus AV = 2.9 ± 0.1). We investigate the origin of the strong dust attenuation and find indications that these K-faint galaxies have smaller dust continuum sizes than the KAB ≤ 25.3 mag galaxies, as measured by ALMA, which suggests their high attenuation is related to their compact sizes. We identify a correlation of dust attenuation with star formation rate surface density (SFR), with the K-faint SMGs representing the higher SFR and highest AV galaxies. The concentrated, intense star formation activity in these systems is likely to be associated with the formation of spheroids in compact galaxies at high redshifts, but as a result of their high obscuration these galaxies are completely missed in ultraviolet, optical, and even near-infrared surveys.
|Full text:||(VoR) Version of Record|
Available under License - Creative Commons Attribution 4.0.
Download PDF (1488Kb)
|Publisher Web site:||https://doi.org/10.1093/mnras/stab283|
|Publisher statement:||2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited|
|Date accepted:||28 January 2021|
|Date deposited:||16 September 2021|
|Date of first online publication:||03 February 2021|
|Date first made open access:||16 September 2021|
Save or Share this output
|Look up in GoogleScholar|